How a Plastic Model of the Moon Was Made

Total Page:16

File Type:pdf, Size:1020Kb

How a Plastic Model of the Moon Was Made --a"1 ---ZFT ----'wo -sy-" --;- '0-; ms"crz ;v-ac' ""m7�- -'tnT�r-z wz'rs3a�zt� G 68 SCIENTIFIC AMERICAN SUPPLEMENT No. 2013 August 1, 1914 ' The moon, 8 Yz days old, as seen First quarter, as seen on the Last quarter, as seen on the sculp­ The moon, 20 Yz days old, as seen through the telescope. sculptured moon. tured model. through the teles�ope. How a Plastic Model of the Moon Was Made The Hemisphere of the Moon Constructed After Telescopic Photographs By Herbert Collier AFTER some years of telescopic observation with a blurry confusion in the fierce light of overhead rays. In undertook the systematic photographing of the moon. A Brashear telescope I determined to undertake the task such a moving picture there is a peculiar fascination. unique telescope was designed, and elaborate plans and of sculpturing the moon, mainly for the, purpose of at­ A new panorama presents itself each night to the watch­ specifications made for this remarkable undertaking. taining greater familiarity personally with every detail ful eye. To see it all is impossible, as the moon is in The instrument was an ingenious combination of a huge of the surface. the visible sky for but a few hours comparatively, and object-glass or light collector nearly two feet in diam­ When you consider that the artist's model was some nightly vigils with the telescope are sure to be inter­ eter and mirrors. Equatorially mounted and�driven by 240,000 miles away and had gained a reputation rupted frequently by cloudy weather or bad atmos­ clockwork, the refracting lens faithfully followed the through the ages of being "fickle," some of the difficul­ pheric conditions. Thus a long course of looking is ob­ object across the sky, while the mirrors, two in num­ ties become apparent. Every day the moon has a dif­ ligatory before the student by personal observation ber, were so arranged as to convey the image thus se­ ferent appearance-a new dress every sitting. As the knows the surface of the moon thoroughly. cured through a tube in the wall to the eye-piece situ­ sunlight creeps over the hills and lights up the moun­ Though my eye had registered through the telescope ated within a comfortable room. Here the camera was taiu peaks, the view of yesterday changes, and quite a thousands of impressions of the surface markings of attached, and the 'men worked free from the usual new aspect results. New valleys, great yawning craters the moon, I dared not trust that organ solely in trans­ bodily discomforts associated with the ordinary tele­ jump into view with their dark depths untouched by ferring them to sculpture.' Accuracy of result de­ scope. even a glimmer of twilight, forming a background of manded exact measurements. Telescopic photographs While some of the finest individual photographs of Rembrandt's choosing. Continually the terminator, the present an unchanging recorq. They give an indelible the moon have been taken by the great telescope at the irregular dawn line dividing light and darkness, is impression of what is revea:�ed, and such permanent Yerkes Observatory, which is the largest refracting tele­ moving forward. On the earth this travels at the rate record is ready for investigation at all times. Beyond scope in the world, nothing can Compare with the series of about 1,000 miles an hour, completing the circuit of question, photography pr,e-emi'i.tently has enabled astron­ secured by the Paris astronomers through years of de­ the globe in one day:' On the moon this movement is omy to merit the title given ,it to-day "the most exact voted effort. Thousands of photographs were taken of about 225 miles per diy, or nearly 10 miles an hour, for of sciences." Therefore- I made, as the foundation of the moon at all stages of its progress from new to full, the earth turns round 29% times to one revolution of my work, the best series of photographs of the moon and then on to new again. Possibly twenty would be the moon. that the world has to-day, which is known as the Paris secured one night and but one selected as good enough The details of cr3{ters-breadth and depth, a crag Atlas. to enter the atlas. These pictures form a wonderful here, a precipice then�--show clearly, contrasted by the Twenty years ago M. Loewy, the gifted director of catalogue of the topography of the moon, presenting far shadows. But as thi sun rises all this passes into the Paris Observatory, with his colleague, M. Puiseux, more minute details of the surface of our own satellite Full moon as seen in the telescopes. Full moon as it appears on the model, © 1914 SCIENTIFIC AMERICAN, INC August 1, 1914 SCIENTIFIC AMERICAN SUPPLEMENT No. 2013 69 1 Kastner 78 Bianchini NAMES CORRESPONDING TO KEY-MAP, LOCATING ALL PROMINENT OBJECTS ON THE MOON. 452 Burg 604 Epigenes 2 Maclaurin 79 Playfair 453 Plana 605 Fontenelli 3 Lapeyrouse 80 Fermat 220 Wargentin 256 Pictet 292 Purbach 416 Hahn 454 Posidonins 606 Anaximenes 4 Ansger 81 Pons 221 Weigel 257 Nasireddin 293 Lacaille 417 Berosus 455 ' Chacornac 607 Carpenter 5 Behaim 82 Azophi 222 Riist 258 Miller 294 Delaunay 418 Burckhardt 456 Romer 608 J. Herschel 6 Hecataus 83 Abenezra 223 Schiller 259 Sasserides 295 Thebit 419 Gauss 457 Macroibus 609 Anaximander 7 Philips 84 Donati 224 Bayer 260 Wilhelm I. 296 Right Wall 420 Geminus 458 Proclus 610 Pythagoras 8 Legendre 85 Faye 225 Schickard 261 Heinsius 297 Arzachel 421 Berzelius 459 Taruntius 611 South 9 Haze 86 Almanon 226 Inghirami 262 Hainzel 298 Alphonsus 422 Messala 460 Maskelyne 612 Harpalus 10 Furnerius 87 Catharina 227 Lehmann Bouvard 263 Lexell 299 ptolemaus 423 Franklin 461 Sabine 613 Xenophenes 11 Marinus 88 Cyrillus 228 Drebbel 264 Hell 300 Wm. Herschel 424 Cepheus 462 Ritter 614 Plato 12 Oken 89 Theophilus 229 265 Gauricus 301 Alpetragius 425 Oersted 463 Arago 615 Plato A. 13 Fraunhofer 90 Beaumont 230 Clausius 266 Wurzel bauer 302 Lassell 426 Volta 464 Sosigenes 6J6 Condamine 14 Brisbane 91 Madler 231 Lacroix 267 Pitatus 303 Davy 427 Long 465 Godin 617 Bouguer 15 Hannon 92 Torricelli 232 Piazzi 268 Hesiodus 304 Lalande 428 Mercurius 466 Rhaeticus 618 Straight Range 16 Pentecoulant 93 Hypatia 233 Lagrange 269 Cichus 305 Flammarion 429 Endymion 467 Tresnecker 619 Cape Laplace 17 Biela 94 Delambre 468 Agrippa 620 Cape Heraclides 18 Hagecius 95 Taylor Soul' H 469 Ukert 621 Bianchini 19 Helmholz 96 Kant 470 Hyginus 622 Sharp 20 Boussillgault 97 Descart�s . 471 Boscovich 623 Mairan 21 Boguslawsky 98 Abulfeda 624 Repsold 22 Manzinus 99 Hipparc'hus 625 Harding 23 Mutus 100 Albategnius 626 Gerard 24 Simpelius $27 Lavoisier 25 Curtius 628 Ulugh Beigh 26 Pentland 629 Lich ten berg 27 Zach 630 Otto Struve 28 Jacobi 631 Aristarchus 29 Lilius 632 Herodotus 30 Cuvier 633 Schiaparelli 31 Bacon 634 Seleucus 32 Pitiscus Kraft 33 Rosenberger 34 Vlacq 35 Steinheil 36 Janssen (S) 37 Fabricus 38 Metius 39 Rheita 40 Stevinus 636 Cardanus 41 Snellius 637 Galileo 42 Reichenbach 638 Marinus 43 Petavius 639 Reiner 44 Vendelinus 640 Olbers 45 Langrenus 641 Hevel 46 Webb 642 East 47 Messier ,643 Encke 48 Goclenius 101 Hind 475 Ross 644 Kepler 49 Guttenberg 102 Halley 476 Plinius 645 Kunowsky 50 Capella 103 Argelander 477 Jansen 646 Reinhold 51 Isidorus 104 Airy 478 Dawes '647 Copernicus 52 Colombo 105 Reaumur 479 Vitruvius 648 Gay-Lussac 53 Cook 106 Sacrobosco 480 Maraldi 649 Tobias Mayer 54 Santbech 107 Schamberger 481 Argaeus Mts. ,650 Euler 55 Bohnenberger 108 Janssen 482 Lemonnier 651 Diophantus 56 Fracastorius 109 Horrocks 234 Fourier 270 Capuanus 306 Masting 4:lO Atlas 483 Bessel 652 Delisle 57 Borda 110 Rothmann 235 Vieta 271 Ramsden 307 Birt 431 Hercules 484 Aratus 653 Gruithuisell 58 Neander 111 Lindenau 236 Palmieri 272 Vitello 308 Prom. Aenarium 432 De la Rue 485 Linne 654 Helicon 59 Picclomini 201 Newton 237 Cavendish 273 Mercator 3()9 Huggins 433 Strabo 486 Conon 655 Lavoisier 60 Stiborius 202 Moretus 238 Henry 274 Campanus 310 Liebig 434 Thales 487 Autolycus 656 Mt. Pico 61 Riccius 203 Cysatus 239 Byrgius 275 Kies 311 Lee 435 Democritus 488 Aristillus 657 Mt, Piton 62 Rabbi Levi 204 Casalus 240 Darwin 2'16 Doppelmayer 312 Hippalus 436 Kant 489 Theaetetus 658 Kirch 6:3 Zagut 205 Klaproth 241 Zupus 277 Mersenius 401 Schubert 437 Moigno 490 Cassini 659 Archimedes 64 Nicolai 206 Wilson 242 Fontana 278 Gassendi 402 Apollonius 438 Euctemon 491 Prot agoras 660 Timocharis 65 Biishing 207 Blancanus 243 Criiger 279 Letronne 403 Neper 439 Challis 492 Peirce 661 Lambert 66 Buch 208 Scheiner 244 Sirsalis 280 Billy 404 Firmin 440 Gioja 493. Eernouilli 662 Pytheas , 67 Maurolycus 209 Gruemberger 245 Trouvelot 2'81 Hansteen 405 Condorcet 441 Barrow 494" Timaeus 663 Eratosthenes 68 Barocius 210 Clavius 246 Rocca 282 Flamsteed 406 Auzout 442 W. C. Bond 495 Scoresby 664 Stadius 69 Licetus 211 Deluc 247 Grimaldi 283 Landsberg 407 Hansen 443 Ch. Mayer 496 Goldschmidt 665 Pallas 70 Stotler 212 Kircher 248 Damoiseau 284 Fra Mauro 408 Picard 444 Archytas 497 Meton 666 Schroter 71 Fernelius 213 Bettinus 249 Riccioli 285 Bonpland 409 Cape Agarum 445 Alpine Valley 498 Kirchhoff 667 S6mmering 72 Frisius 214 Bailly 250 Lohrmann 286 Pamy 410 Alhazen 446 Aristoteles 499 Schumacher 668 Gambart 73 Pont anus 215 Zuchius 251 Maginus 287 Guerike 411 Eimmart 447 Egede GOO Hooke 669 Briggs 74 AliacensiR 216 Segner 252 LongolllOntanl1S 288 L u biniezky 412 Oriani 44i1 EuejoxeR 1i0! ('",sar 670 Cava ]�l'inR 75 Walter 217 Yausen 253 Street 289 Bullialdus 413 Plutarch 449 Alexander 6()1 Anaxag01'3F1 ti71 Rainbow Bay 76 Werner 218 Procylides 254 Saussure 290 Agatharchides 414 Cleomedes 450 Calippus 602 Philolaus 672 Maupertius 77 Apian 219 Nasmytll 255 Tycho 291 Regiomontanus 415 Tralles 451 Baily 603 Birmingham 673 Foucault © 1914 SCIENTIFIC AMERICAN, INC 70 SCIENTIFIC AMERICAN SUPPLEMENT No.
Recommended publications
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • Glossary Glossary
    Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts.
    [Show full text]
  • General Index
    General Index Italicized page numbers indicate figures and tables. Color plates are in- cussed; full listings of authors’ works as cited in this volume may be dicated as “pl.” Color plates 1– 40 are in part 1 and plates 41–80 are found in the bibliographical index. in part 2. Authors are listed only when their ideas or works are dis- Aa, Pieter van der (1659–1733), 1338 of military cartography, 971 934 –39; Genoa, 864 –65; Low Coun- Aa River, pl.61, 1523 of nautical charts, 1069, 1424 tries, 1257 Aachen, 1241 printing’s impact on, 607–8 of Dutch hamlets, 1264 Abate, Agostino, 857–58, 864 –65 role of sources in, 66 –67 ecclesiastical subdivisions in, 1090, 1091 Abbeys. See also Cartularies; Monasteries of Russian maps, 1873 of forests, 50 maps: property, 50–51; water system, 43 standards of, 7 German maps in context of, 1224, 1225 plans: juridical uses of, pl.61, 1523–24, studies of, 505–8, 1258 n.53 map consciousness in, 636, 661–62 1525; Wildmore Fen (in psalter), 43– 44 of surveys, 505–8, 708, 1435–36 maps in: cadastral (See Cadastral maps); Abbreviations, 1897, 1899 of town models, 489 central Italy, 909–15; characteristics of, Abreu, Lisuarte de, 1019 Acequia Imperial de Aragón, 507 874 –75, 880 –82; coloring of, 1499, Abruzzi River, 547, 570 Acerra, 951 1588; East-Central Europe, 1806, 1808; Absolutism, 831, 833, 835–36 Ackerman, James S., 427 n.2 England, 50 –51, 1595, 1599, 1603, See also Sovereigns and monarchs Aconcio, Jacopo (d. 1566), 1611 1615, 1629, 1720; France, 1497–1500, Abstraction Acosta, José de (1539–1600), 1235 1501; humanism linked to, 909–10; in- in bird’s-eye views, 688 Acquaviva, Andrea Matteo (d.
    [Show full text]
  • Feature of the Month – January 2016 Galilaei
    A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – JANUARY 2016 GALILAEI Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA October 26, 2015 03:32-03:58 UT, 15 cm refl, 170x, seeing 8-9/10 I sketched this crater and vicinity on the evening of Oct. 25/26, 2015 after the moon hid ZC 109. This was about 32 hours before full. Galilaei is a modest but very crisp crater in far western Oceanus Procellarum. It appears very symmetrical, but there is a faint strip of shadow protruding from its southern end. Galilaei A is the very similar but smaller crater north of Galilaei. The bright spot to the south is labeled Galilaei D on the Lunar Quadrant map. A tiny bit of shadow was glimpsed in this spot indicating a craterlet. Two more moderately bright spots are east of Galilaei. The western one of this pair showed a bit of shadow, much like Galilaei D, but the other one did not. Galilaei B is the shadow-filled crater to the west. This shadowing gave this crater a ring shape. This ring was thicker on its west side. Galilaei H is the small pit just west of B. A wide, low ridge extends to the southwest from Galilaei B, and a crisper peak is south of H. Galilaei B must be more recent than its attendant ridge since the crater's exterior shadow falls upon the ridge.
    [Show full text]
  • Optics, Basra, Cairo, Spectacles
    International Journal of Optics and Applications 2014, 4(4): 110-113 DOI: 10.5923/j.optics.20140404.02 Alhazen, the Founder of Physiological Optics and Spectacles Nāsir pūyān (Nasser Pouyan) Tehran, 16616-18893, Iran Abstract Alhazen (c. 965 – c. 1039), Arabian mathematician and physicist with an unknown actual life who laid the foundation of physiological optics and came within an ace of discovery of the use of eyeglasses. He wrote extensively on algebra, geometry, and astronomy. Just the Beginnings of the 13th century, in Europe eyeglasses were used as an aid to vision, but Alhazen’s book “Kitab al – Manazir” (Book of Optics) included theories on refraction, reflection and the study of lenses and gave the first account of vision. It had great influence during the Middle Ages. In it, he explained that twilight was the result of the refraction of the sun’s rays in the earth’s atmosphere. The first Latin translation of Alhazen’s mathematical works was written in 1210 by a clergyman from Sussex, in England, Robert Grosseteste (1175 – 1253). His treatise on astrology was printed in Latin at Basle in 1572. Alhazen who was from Basra died in Cairo at the age of 73 (c. 1039). Keywords Optics, Basra, Cairo, Spectacles Ibn al-Haytham (c. 965 – c. 1038), known in the West who had pretended insane, once more was released from the Alhazen, and Avenna than1, who is considered as the father prison and received his belongings, and never applied for any of modern optics. He was from Basra [1] (in Iraq) and position. received his education in this city and Baghdad, but nothing is known about his actual life and teachers.
    [Show full text]
  • Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography on the Occasion of the 50Th Anniversary of Apollo 11 Moon Landing
    Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography On the occasion of the 50th anniversary of Apollo 11 moon landing Please note: A specific item in this catalogue may be sold or is on hold if the provided link to our online inventory (by clicking on the blue-highlighted author name) doesn't work! Milestones of Science Books phone +49 (0) 177 – 2 41 0006 www.milestone-books.de [email protected] Member of ILAB and VDA Catalogue 07-2019 Copyright © 2019 Milestones of Science Books. All rights reserved Page 2 of 71 Authors in Chronological Order Author Year No. Author Year No. BIRT, William 1869 7 SCHEINER, Christoph 1614 72 PROCTOR, Richard 1873 66 WILKINS, John 1640 87 NASMYTH, James 1874 58, 59, 60, 61 SCHYRLEUS DE RHEITA, Anton 1645 77 NEISON, Edmund 1876 62, 63 HEVELIUS, Johannes 1647 29 LOHRMANN, Wilhelm 1878 42, 43, 44 RICCIOLI, Giambattista 1651 67 SCHMIDT, Johann 1878 75 GALILEI, Galileo 1653 22 WEINEK, Ladislaus 1885 84 KIRCHER, Athanasius 1660 31 PRINZ, Wilhelm 1894 65 CHERUBIN D'ORLEANS, Capuchin 1671 8 ELGER, Thomas Gwyn 1895 15 EIMMART, Georg Christoph 1696 14 FAUTH, Philipp 1895 17 KEILL, John 1718 30 KRIEGER, Johann 1898 33 BIANCHINI, Francesco 1728 6 LOEWY, Maurice 1899 39, 40 DOPPELMAYR, Johann Gabriel 1730 11 FRANZ, Julius Heinrich 1901 21 MAUPERTUIS, Pierre Louis 1741 50 PICKERING, William 1904 64 WOLFF, Christian von 1747 88 FAUTH, Philipp 1907 18 CLAIRAUT, Alexis-Claude 1765 9 GOODACRE, Walter 1910 23 MAYER, Johann Tobias 1770 51 KRIEGER, Johann 1912 34 SAVOY, Gaspare 1770 71 LE MORVAN, Charles 1914 37 EULER, Leonhard 1772 16 WEGENER, Alfred 1921 83 MAYER, Johann Tobias 1775 52 GOODACRE, Walter 1931 24 SCHRÖTER, Johann Hieronymus 1791 76 FAUTH, Philipp 1932 19 GRUITHUISEN, Franz von Paula 1825 25 WILKINS, Hugh Percy 1937 86 LOHRMANN, Wilhelm Gotthelf 1824 41 USSR ACADEMY 1959 1 BEER, Wilhelm 1834 4 ARTHUR, David 1960 3 BEER, Wilhelm 1837 5 HACKMAN, Robert 1960 27 MÄDLER, Johann Heinrich 1837 49 KUIPER Gerard P.
    [Show full text]
  • Exploration of the Moon
    Exploration of the Moon The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959. Prior to that the only available means of exploration had been observation from Earth. The invention of the optical telescope brought about the first leap in the quality of lunar observations. Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it. NASA's Apollo program was the first, and to date only, mission to successfully land humans on the Moon, which it did six times. The first landing took place in 1969, when astronauts placed scientific instruments and returnedlunar samples to Earth. Apollo 12 Lunar Module Intrepid prepares to descend towards the surface of the Moon. NASA photo. Contents Early history Space race Recent exploration Plans Past and future lunar missions See also References External links Early history The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former. His non-religious view of the heavens was one cause for his imprisonment and eventual exile.[1] In his little book On the Face in the Moon's Orb, Plutarch suggested that the Moon had deep recesses in which the light of the Sun did not reach and that the spots are nothing but the shadows of rivers or deep chasms.
    [Show full text]
  • DMAAC – February 1973
    LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base.
    [Show full text]
  • August 2017 Posidonius P & Luther
    A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – AUGUST 2017 POSIDONIUS P & LUTHER Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 5, 2017 01:28-01:48; UT, 15 cm refl, 170x, seeing 7-8/10. I drew these craters on the evening of March 4/5, 2017 while the moon was hiding some Hyades stars. This area is in northeast Mare Serenitatis west of Posidonius itself. Posidonius P is the largest crater on this sketch. The smaller crater south of P is Posidonius F and Posidonius G is the tiny pit to the north. There is a halo around Posidonius G, but this crater is noticeably north of the halo's center. A very low round swelling is northeast of Posidonius G. Luther is the crater well to the west of Posidonius P. All four of these craters are crisp, symmetric features, differing only in size. There are an assortment of elevations near Luther. The peak Luther alpha is well to the west of Luther, and showed dark shadowing at this time. All of the other features near Luther are more subtle than Luther alpha. One mound is between Luther and Luther alpha. Two more mounds are north of Luther, and a low ridge is just east of this crater. A pair of very low mounds are south of Luther. These are the vaguest features depicted here, and may be too conspicuous on the sketch.
    [Show full text]
  • The Moon After Apollo
    ICARUS 25, 495-537 (1975) The Moon after Apollo PAROUK EL-BAZ National Air and Space Museum, Smithsonian Institution, Washington, D.G- 20560 Received September 17, 1974 The Apollo missions have gradually increased our knowledge of the Moon's chemistry, age, and mode of formation of its surface features and materials. Apollo 11 and 12 landings proved that mare materials are volcanic rocks that were derived from deep-seated basaltic melts about 3.7 and 3.2 billion years ago, respec- tively. Later missions provided additional information on lunar mare basalts as well as the older, anorthositic, highland rocks. Data on the chemical make-up of returned samples were extended to larger areas of the Moon by orbiting geo- chemical experiments. These have also mapped inhomogeneities in lunar surface chemistry, including radioactive anomalies on both the near and far sides. Lunar samples and photographs indicate that the moon is a well-preserved museum of ancient impact scars. The crust of the Moon, which was formed about 4.6 billion years ago, was subjected to intensive metamorphism by large impacts. Although bombardment continues to the present day, the rate and size of impact- ing bodies were much greater in the first 0.7 billion years of the Moon's history. The last of the large, circular, multiringed basins occurred about 3.9 billion years ago. These basins, many of which show positive gravity anomalies (mascons), were flooded by volcanic basalts during a period of at least 600 million years. In addition to filling the circular basins, more so on the near side than on the far side, the basalts also covered lowlands and circum-basin troughs.
    [Show full text]
  • Meet the Philosophers of Ancient Greece
    Meet the Philosophers of Ancient Greece Everything You Always Wanted to Know About Ancient Greek Philosophy but didn’t Know Who to Ask Edited by Patricia F. O’Grady MEET THE PHILOSOPHERS OF ANCIENT GREECE Dedicated to the memory of Panagiotis, a humble man, who found pleasure when reading about the philosophers of Ancient Greece Meet the Philosophers of Ancient Greece Everything you always wanted to know about Ancient Greek philosophy but didn’t know who to ask Edited by PATRICIA F. O’GRADY Flinders University of South Australia © Patricia F. O’Grady 2005 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise without the prior permission of the publisher. Patricia F. O’Grady has asserted her right under the Copyright, Designs and Patents Act, 1988, to be identi.ed as the editor of this work. Published by Ashgate Publishing Limited Ashgate Publishing Company Wey Court East Suite 420 Union Road 101 Cherry Street Farnham Burlington Surrey, GU9 7PT VT 05401-4405 England USA Ashgate website: http://www.ashgate.com British Library Cataloguing in Publication Data Meet the philosophers of ancient Greece: everything you always wanted to know about ancient Greek philosophy but didn’t know who to ask 1. Philosophy, Ancient 2. Philosophers – Greece 3. Greece – Intellectual life – To 146 B.C. I. O’Grady, Patricia F. 180 Library of Congress Cataloging-in-Publication Data Meet the philosophers of ancient Greece: everything you always wanted to know about ancient Greek philosophy but didn’t know who to ask / Patricia F.
    [Show full text]
  • THE STUDY of SATURN's RINGS 1 Thesis Presented for the Degree Of
    1 THE STUDY OF SATURN'S RINGS 1610-1675, Thesis presented for the Degree of Doctor of Philosophy in the Field of History of Science by Albert Van Haden Department of History of Science and Technology Imperial College of Science and Teohnology University of London May, 1970 2 ABSTRACT Shortly after the publication of his Starry Messenger, Galileo observed the planet Saturn for the first time through a telescope. To his surprise he discovered that the planet does.not exhibit a single disc, as all other planets do, but rather a central disc flanked by two smaller ones. In the following years, Galileo found that Sa- turn sometimes also appears without these lateral discs, and at other times with handle-like appendages istead of round discs. These ap- pearances posed a great problem to scientists, and this problem was not solved until 1656, while the solution was not fully accepted until about 1670. This thesis traces the problem of Saturn, from its initial form- ulation, through the period of gathering information, to the final stage in which theories were proposed, ending with the acceptance of one of these theories: the ring-theory of Christiaan Huygens. Although the improvement of the telescope had great bearing on the problem of Saturn, and is dealt with to some extent, many other factors were in- volved in the solution of the problem. It was as much a perceptual problem as a technical problem of telescopes, and the mental processes that led Huygens to its solution were symptomatic of the state of science in the 1650's and would have been out of place and perhaps impossible before Descartes.
    [Show full text]